A Study of the Lunar Subsurface Echo Intensity for Evaluation of the Maximum Detection Depth of the Kaguya Lunar Radar Sounder

Details A Study of the Lunar Subsurface Echo Intensity for Evaluation of the Maximum Detection Depth of the Kaguya Lunar Radar Sounder A Study of the Lunar Subsurface Echo Intensity for Evaluation of the Maximum Detection Depth of the Kaguya Lunar Radar Sounder

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1465k&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1465

Physics

Scientific paper

The lunar subsurface echo power was estimated based on the reflectance
at the buried regolith layers and attenuation rate in the basalt lava
flow layers. The maximum detection depth of Kaguya/LRS was also
evaluated based on it.

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